Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Paul A. Vanden Bout"'
Autor:
Ronald J. Maddalena, Rob Ivison, David T. Frayer, Andrew Blain, Ian Smail, Paul A. Vanden Bout
Publikováno v:
Astrophysical journal, 2018, Vol.860(2), pp.87 [Peer Reviewed Journal]
Frayer, D T, Maddalena, R J, Ivison, R J, Smail, I, Blain, A W & Bout, P V 2018, ' The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136 ', Astrophysical Journal, vol. 860, no. 2, 87 . https://doi.org/10.3847/1538-4357/aac49a
Frayer, D T, Maddalena, R J, Ivison, R J, Smail, I, Blain, A W & Bout, P V 2018, ' The Discovery of a New Massive Molecular Gas Component Associated with the Submillimeter Galaxy SMM J02399-0136 ', Astrophysical Journal, vol. 860, no. 2, 87 . https://doi.org/10.3847/1538-4357/aac49a
We present CO(1-0), CO(3-2), and CO(7-6) observations using the Green Bank Telescope (GBT) and the Atacama Large Millimeter Array (ALMA) of the z=2.8 sub-millimeter galaxy SMM J02399-0136. This was the first submillimeter-selected galaxy discovered a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3077e8210c82e73b986e5165802bf5ef
http://dro.dur.ac.uk/25376/
http://dro.dur.ac.uk/25376/
Autor:
Min Yun, Roberto Decarli, Catherine Vlahakis, Christopher C. Hayward, Joshua E. Barnes, Fabian Walter, Brant Robertson, Paul Torrey, Jin Koda, Lena Murchikova, Paul A. Vanden Bout, Reinhard Genzel, Lee Armus, Lars Hernquist, Todd A. Thompson, David B. Sanders, Phil Hopkins, Laura K. Zschaechner, Pierre Cox, Paul van der Werf, Nick Scoville, Kartik Sheth, Linda J. Tacconi
Publikováno v:
ASTROPHYSICAL JOURNAL (ISSN 0004-637X), 836, 66
ASTROPHYSICAL JOURNAL (ISSN 0004-637X)
NASA Astrophysics Data System
ASTROPHYSICAL JOURNAL (ISSN 0004-637X)
NASA Astrophysics Data System
We present 90 mas (37 pc) resolution ALMA imaging of Arp 220 in the CO (1-0) line and continuum at $\lambda = 2.6$ mm. The internal gas distribution and kinematics of both galactic nuclei are well-resolved for the first time. In the West nucleus, the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd363e14ac1cb3bb5f7b445503b9151d
http://hdl.handle.net/20.500.12386/30231
http://hdl.handle.net/20.500.12386/30231
Publikováno v:
The Astrophysical Journal. 707:988-999
We report observations of 15 high redshift (z = 1-5) galaxies at 350 microns using the Caltech Submillimeter Observatory and SHARC-II array detector. Emission was detected from eight galaxies, for which far-infrared luminosities, star formation rates
Publikováno v:
Physics Today. 70:71-71
Radio astronomer and physicist Kwok-Yung “Fred” Lo was born on 19 October 1947 in Nanjing, China. The third of six sons, he grew up in Hong Kong, where his father had moved his antique business in 1949 in search of better opportunities. Fred came
Autor:
Paul A. Vanden Bout
Publikováno v:
Physics Today. 68:69-69
Publikováno v:
Physics Today. 44:41-49
Radioastronomy began in 1933 with Karl Jansky's accidental discovery of radio emission from the center of the Galaxy as he was studying the effect of thunderstorms on transatlantic telecommunications. Six decades later, telecommunications and other r
Autor:
Paul A. Vanden Bout
Publikováno v:
Advances in Space Research. 11:387-395
Autor:
Robert L. Brown, Paul A. Vanden Bout
Publikováno v:
The Structure and Content of Molecular Clouds 25 Years of Molecular Radioastronomy ISBN: 9783540586210
The prospects for molecular astrophysics at high redshifts are presented. The discussion is concentrated on the sources IRAS 10214+4724.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::052f9b97255e8e0e892469b52a31d521
https://doi.org/10.1007/3540586210_24
https://doi.org/10.1007/3540586210_24
We present here the sensitive HCN(1-0) observations made with the VLA of two submillimeter galaxies and two QSOs at high-redshift. HCN emission is the signature of dense molecular gas found in GMC cores, the actual sites of massive star formation. We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd4223a841f3502d3cae58ac480e9dc0
Observations have revealed prodigious amounts of star formation in starburst galaxies as traced by dust and molecular emission, even at large redshifts. Recent work shows that for both nearby spiral galaxies and distant starbursts, the global star fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb68dcfc4bc48febedd5015d748a7ab7
http://arxiv.org/abs/astro-ph/0511424
http://arxiv.org/abs/astro-ph/0511424